In this study, we prioritized the stars that have precise spectroscopic, astrometric and photometric data in the literature. In this context, we used the spectroscopic data from 14 studies [1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, [8]}, [9]}, [10]}, [11]}, [12]}, [13]}, [14]}. 6149 stars with atmospheric model parameters (\(T_{eff}\) , \(\log g\)  and [Fe/H]) could be provided from these studies (Table 1). The photometric data are supplied from GALEX DR7 [15]} and UBV [16]}, [17]}, [18]}, [19]}, [20]}, [21]}, while the trigonometric parallaxes are taken from Gaia DR2 [22]}. The photometric and astrometric data of 5593 stars were not available for the original set of stars (6149 stars). Hence, our sample reduced to 556 (Table 2).
